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GEOPHYSICAL RESEARCH LETTERS,
VOL. 33,
L12S02,
doi:10.1029/2006GL025770,
2006
The effect of pressure on the structure and volume of ferromagnesian post-perovskite
Wendy L. Mao
Los Alamos Neutron Science Center, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
Ho-kwang Mao
Geophysical Laboratory, Carnegie Institution of Washington, Washington, D. C., USA
Vitali B. Prakapenka
GeoSoilEnviroCARS, University of Chicago, Chicago, Illinois, USA
Jinfu Shu
Geophysical Laboratory, Carnegie Institution of Washington, Washington, D. C., USA
Russell J. Hemley
Geophysical Laboratory, Carnegie Institution of Washington, Washington, D. C., USA
Abstract
We determined pressure-volume (P-V) data for (Mg0.6Fe0.4)SiO3 post-perovskite (ppv) upon decompression from 140 GPa. The data can be divided into four regions: above 95 GPa, diffraction
peaks are sharp and follow a smooth and tight P-V curve; below 90 GPa, peak widths increase, and a kink develops in the P-V curve; below 60 GPa, the broadening plateaus; below 4.6 GPa, the ppv pattern disappears. This suggests that defects and stacking
faults start to develop in ppv at 90 GPa and saturate at 60 GPa, and the structure disintegrates below 4.6 GPa. The volume
and density of the (Mg0.6Fe0.4)SiO3 ppv is well constrained by our data at the pressures relevant to the Earth's D″ layer. Our bulk modulus in this region is
much higher than theoretical calculations for pure MgSiO3 ppv.
Received 13
January
2006;
accepted 27
March
2006;
published 5
May
2006.
Index Terms: 3919 Mineral Physics: Equations of state; 3924 Mineral Physics: High-pressure behavior; 3954 Mineral Physics: X-ray, neutron, and electron spectroscopy and diffraction.
Subscriber Access to Full Article (Nonsubscribers may purchase for $9.00, Includes print PDF, file size: 184133 bytes)
Citation: Mao, W. L., H. Mao, V. B. Prakapenka, J. Shu, and R. J. Hemley
(2006),
The effect of pressure on the structure and volume of ferromagnesian post-perovskite,
Geophys. Res. Lett.,
33,
L12S02,
doi:10.1029/2006GL025770.
Copyright 2006 by the American Geophysical Union.
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